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Physics LibreTexts

3: Kinematics

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At this stage, many students raise the following questions, which turn out to be related to one another:

  1. According to Einstein, if observers A and B aren’t at rest relative to each other, then A says B’s time is slow, but B says A is the slow one. How can this be? If A says B is slow, shouldn’t B say A is fast? After all, if I took a pill that sped up my brain, everyone else would seem slow to me, and I would seem fast to them.
  2. Suppose I keep accelerating my spaceship steadily. What happens when I get to the speed of light?
  3. In all the diagrams in Section 1.4, the parallelograms have their diagonals stretched and squished by a certain factor, which depends on v. What is the interpretation of this factor?

  • 3.1: How can they both . . . ?
  • 3.2: The stretch factor is the Doppler shift
    The stretching and squishing factors for the diagonals are the same as the Doppler shift. We notate this factor as D (which can stand for either “Doppler” or “diagonal”).
  • 3.3: Combination of Velocities
    In nonrelativistic physics, velocities add in relative motion. For example, if a boat moves relative to a river, and the river moves relative to the land, then the boat’s velocity relative to the land is found by vector addition. This linear behavior cannot hold relativistically.
  • 3.4: No frame of reference moving at c
    No continuous process of acceleration can boost a material object to c . That is, the subluminal (slower than light) nature of a electron or a person is a fundamental feature of its identity and can never be changed. Einstein can never get on his motorcycle and drive at c as he imagined when he was a young man, so we material beings can never see the world from a frame of reference that travels at c.
  • 3.5: The Velocity and Acceleration Vectors
  • 3.6: Some kinematic identities
    The following identities can be handy. If stranded on a desert island you should be able to rederive them from scratch. Don’t memorize them.
  • 3.7: The Projection Operator
    A frequent source of confusion in relativity is that we write down equations that are coordinate-dependent, but forget the dependency. Similarly, it is possible to write expressions that are only valid for one choice of signature. The following notation, defining a projection operator P , is one tool for avoiding these difficulties.
  • 3.8: Faster-than-light frames of reference?
    Special relativity doesn’t permit the existence of observers who move at c . This is because if two observers differ in velocity by c , then the Lorentz transformation between them is not a one-to-one map, which is physically unacceptable.
  • 3.9: Thickening of a curve
  • 3.E: Kinematics (Exercises)


This page titled 3: Kinematics is shared under a CC BY-SA 4.0 license and was authored, remixed, and/or curated by Benjamin Crowell via source content that was edited to the style and standards of the LibreTexts platform.

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